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Table 1
Characterization of the observed fields.
Field name | l | b | SN | E(J − K) | N stars | %Giants |
|
||||||
p1m4 | 1 | −4 | 90 | 0.21 | 321 | 98 |
p0m6 | 0 | −6 | 82 | 0.14 | 227 | 98 |
m1m10 | −1 | −10 | 101 | 0.06 | 227 | 74 |
p7m9 | 7 | −9 | 81 | 0.11 | 223 | 91 |
m10m8 | −10 | −8 | 98 | 0.06 | 222 | 79 |
Notes. The reddening E(J − K) values are those estimated in Sect. 3. The signal-to-noise ratio is derived from averaging the individual values of all stars in each field.
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